Quantum physics has intrigued scientists and philosophers alike, because it challenges our notions of reality and locality — concepts that we have grown to rely on in our macroscopic world. It is an intriguing open question whether the linearity of quantum mechanics extends into the macroscopic domain. Scientific progress over the past decades inspires hope that this debate may be settled by table-top experiments.
The past three decades have witnessed what has been termed1 the second quantum revolution: a renaissance of research on the quantum foundations, hand in hand with growing experimental capabilities2, revived the idea of exploiting quantum superpositions for technological applications, from information science3,4,5 to precision metrology6,7,8. Quantum mechanics has passed all precision tests with flying colours, but it still seems to be in conflict with our common sense. As quantum theory knows no boundaries, everything should fall under the sway of the superposition principle, including macroscopic objects. This is at the bottom of Schrödinger’s thought experiment of transforming a cat into a state that strikes us as classically impossible. And yet, ‘Schrödinger kittens’ of entangled photons9 and ions10 have been realized in the lab.
So why are the objects around us never found in superpositions of states that would be impossible in a classical description? One may emphasize the smallness of Planck’s constant, or point to decoherence theory, which describes how a system will effectively lose its quantum features when coupled to a quantum environment of sufficient size11,12. The formalism of decoherence, however, is based on the framework of unitary quantum mechanics, implying that some interpretational exercise is required not to become entangled in a multitude of parallel worlds13. More radically, one may ask whether quantum mechanics breaks down beyond a certain mass or complexity scale. As will be discussed below, such ideas can be motivated by the apparent incompatibility of quantum theory and general relativity. It is safe to state, in any case, that quantum superpositions of truly massive, complex objects are terra incognita. This makes them an attractive challenge for a growing number of sophisticated experiments.
We start by reviewing several prototypical tests of the superposition principle, focusing on the quantum states of motion exhibited by material objects. Particle position and momentum variables have a well-defined classical analogue, and they are therefore particularly suited to probe the macroscopic domain. We note that aspects of macroscopicity can also be addressed in experiments with photons14,15,16, with the phonons of ion chains17, and by squeezing pseudospins 8,18.
State of the art
Superconducting quantum interference devices (SQUIDs) have recently attracted a lot of interest, because they are promising elements of quantum information processing19. A SQUID is a superconducting loop segmented by Josephson junctions. Its electronic and transport properties are determined by a macroscopic wavefunction ordering the Cooper pairs. To exploit this macroscopicity it is appealing to consider a flux qubit20 (Fig. 1a): the single-valuedness of the wavefunction means that the magnetic flux encircled by a closed-loop supercurrent must be quantized. In particular, one can define a symmetric and an antisymmetric linear combination of two supercurrents, which circulate simultaneously in opposing directions. Billions of electrons may contribute coherently to the wavefunction over mesoscopic dimensions. The difference between the clockwise and anti-clockwise currents21 can reach about 2 μA, amounting to a local magnetic moment of about 1010 Bohr magnetons. This is an impressive number, which has led to the suggestion that SQUIDs may exhibit the most macroscopic quantum superposition to date. However, ‘only’ a few thousand of the Cooper pairs carrying the different currents are distinguishable22, which points to the need for an objective measure of macroscopicity (Box 1).
Historically, perfect-crystal neutron quantum optics23 made many interference experiments with atoms and photons possible. As the de Broglie wavelength of thermal neutrons is comparable to the lattice constant of silicon, quantum diffraction off the nuclei may split the neutron wavefunction at large angles. As of today, neutron interferometry still realizes the widest delocalization of any massive object24. With an arm separation up to 7 cm, enclosing an area of 80 cm2, it allows one to stick a hand between the two branches of a quantum state that describes a single microscopic particle (Fig. 1b). Even though neutrons are very light neutral particles, they are prime candidates for emergent tests of post-Newtonian gravity at short distances25,26. With an electrical polarizability twenty orders of magnitude smaller than for atoms, neutrons are much less sensitive to electrostatic perturbations, such as charges, patch effects or van der Waals forces.
Much better control and signal to noise can be achieved by using atoms. Atom interferometry (Fig. 1c) started about 30 years ago27,28,29. The development of Raman30 beam-splitters then transformed the tools of basic science into high-precision quantum sensors that split, invert and recombine the atomic wavefunction in three short laser pulses (Fig. 1c). In particular, inertial forces such as gravity and Coriolis forces31,32 have been measured with stunning precision in experiments that also promise new tests of general relativity33.
The mass in these experiments is always limited to that of a single atom, in practice to the caesium mass of 133 amu. A degree of macroscopicity can still be reached in the spatial extension of the wavefunction and in coherence time. The achievable delocalization depends on the momentum transfer in the beam-splitting element, whereas the coherence time is essentially determined by the duration of free fall in the apparatus. Both impressively wide-angle beam splitters34,35 and very long coherence times36 have been demonstrated separately, and been recently combined in an experiment with rubidium atoms, whose wave packets get separated for 2.3 s with a maximal distance of 1.4 cm (ref. 37). Future quantum sensors are expected to increase the sensitivity of quantum metrology by several orders of magnitude. The coherence time grows only with the square root of the device length, so that it will be practically limited to several seconds in Earth-bound devices, even in high-drop towers. Progress in matter-wave beam splitting will depend on improved wavefront control of the beam splitting lasers and other technological breakthroughs. If it were possible to build interferometers of 100 m length with beam-splitters capable of transferring a hundred grating momenta38, atomic matter would be delocalized over distances of metres. Even though designed for testing the effects of general relativity33,39, such experiments would also test the linearity of quantum mechanics40 as well as the homogeneity of spacetime41.
It is frequently suggested that ultra-cold atomic ensembles may serve to test the linearity of quantum physics even better, as all atoms can be described by a joint many-body wavefunction once they are cooled below the phase transition to Bose–Einstein condensation (Fig. 1d). Billions of non-interacting atoms may be united in a quantum degenerate state, which is, however, a product of single-particle states , so that interference of Bose-condensed atoms depends only on the de Broglie wavelength of single atoms. A genuinely entangled many-particle state akin to a Schrödinger cat state would be required to reduce the fringe spacing. Such macroscopic cat states with regard to the particle motion have remained an open challenge, even though entanglement in other degrees of freedom has been demonstrated between dozens of atoms7,8,42. In contrast to that, macromolecules and clusters open a new field involving strongly bound particles with internal temperatures up to 1,000 K. When N atoms are covalently linked into a single molecule they act as a single object in quantum interference experiments. The entire N-atom system is then delocalized over two or more interferometer arms.
Macromolecule interferometry started originally with the far-field diffraction of fullerenes43 and works with high-mass objects in currently two different settings: the Kapitza–Dirac–Tabot–Lau interferometer (KDTLI) and an all-optical interferometer in the time domain with pulsed ionization gratings (OTIMA). Both concepts were developed and implemented at the University of Vienna44,45 and are based on similar ideas. In high-mass matter-wave interference we face de Broglie wavelengths between 10 fm and 10 pm for objects between 1010 and 103amu. This is more than six orders of magnitude smaller than in all experiments with ultra-cold atoms. Macromolecules are not susceptible to established laser cooling techniques, although first steps towards the cavity cooling of 1010amu objects have been taken46,47. The particles therefore start out in rather mixed states, requiring near-field interference schemes48.
The KDTLI interferometer is sketched in Fig. 1e. It accepts a large variety of nanoparticles, because it uses only non-resonant gratings to split (G1), diffract (G2) and probe (G3) matter-waves. The first grating (G1) implements a spatially periodic transmission function. The size of the slits and the separation between G1 and G2 are chosen such that the position–momentum uncertainty in each slit is sufficient to expand each particle’s wavefunction to cover more than two slits in G2 downstream. To achieve this, G1 must be an absorptive mask, here realized as a silicon nitride nanostructure. Grating G2, a non-resonant standing light wave, imprints a spatially periodic phase onto the matter-wave. A near-field resonance effect rephases the wavefunctions to a molecular density pattern at the position of G3. Although one might capture the emerging quantum fringe pattern on a substrate for subsequent high-resolution microscopy49,50, it is often convenient to scan the absorptive mask G3 across the nanopattern: a plot of the number of transmitted particles as a function of the mask’s position reveals the molecular interferogram (Fig. 1e).
In contrast to the KDTLI, an OTIMA interferometer relies on three pulsed gratings that ionize and thus remove the molecules at the anti-nodes of an ultraviolet standing-wave laser beam51. Such all-optical gratings can handle of highly polarizable or polar particles, and their pulsed nature allows us to profit from working in the time domain. All particles exposed to the spatially extended nanosecond laser pulses then see the same grating for the same time, regardless of their velocity. This eliminates numerous dispersive dephasing phenomena, which is particularly beneficial for quantum tests at high masses52,53. KDTLI and OTIMA are ‘universal’ in the sense that they can accept a wide class of different objects and both avoid the detrimental effect of van der Waals forces in G2 by using non-resonant optical beam-splitters.
Experiments in the KDTLI currently hold the mass record in matter-wave interference, with a functionalized tetraphenylporphyrin molecule that combines 810 atoms into one particle with a molecular weight exceeding 10,000 amu (ref. 54). Even at an internal temperature of 500 K this object can be delocalized over a hundred times its own diameter and for more than 1 ms. Very recently, the OTIMA concept has been demonstrated45 with clusters of molecules. It will soon be used to explore quantum coherence at unprecedented masses52. Both interferometers also share a high potential for quantum-assisted metrology targeting internal properties, which reveal themselves in de Broglie experiments owing to the phase shift induced by external fields55,56,57.
Physics beyond the Schrödinger equation?
The experimental tests discussed so far confirm quantum mechanics impressively, as do high-precision spectroscopic measurements58,59 and tests of nonlocality60,61,62. Many physicists take for granted that quantum theory is valid on macroscopic scales, the more so because environmental decoherence explains why macroscopic objects seem to assume the classically distinguished states we observe in our everyday life11,12 (Fig. 2).
Yet, there are good reasons to take seriously the possibility that quantum theory may fail beyond some scale. A compelling one is the difficulty of reconciling quantum theory with the nonlinear laws of general relativity, which treats spacetime as a dynamical entity. Most theories of quantum gravity suggest that there is a minimal observable length scale, often associated with the Planck length. One way to account for this phenomenologically is to postulate modified commutator relations for the canonical observables, which might be testable by monitoring the motion of massive pendulums at the quantum level63,64,65,66,67. The granularity of spacetime might manifest itself also in a fundamentally non-unitary time evolution of the quantum system, which would be observable as an intrinsic decoherence process41,68,69,70.
The alternative that gravity is not to be quantized, but fundamentally described by a classical field, suggests one should extend the Schrödinger equation nonlinearly to account for the gravitational self-interaction71,72. This idea is formalized in the Schrödinger–Newton equation, which can be obtained as the non-relativistic limit of self-gravitating Klein–Gordon fields73. It has been hypothesized that this equation defines the timescale and the basis states of a fundamental collapse mechanism. Indeed, an additional collapse-like stochastic process is required for any such nonlinear extension of the Schrödinger equation to ensure that the time evolution maps any initial state linearly to an ensemble described by a proper density operator. Otherwise an entangled particle pair would admit superluminal signalling — that is, violate causality — because the nonlinearity would imprint the basis of a distant measurement onto the reduced local state74. A gravitationally-inspired nonlinear modification of quantum mechanics75 can be made consistent with causality and observations at the price of a fictitiously large blurring of the involved mass density71.
The best studied nonlinear modification of quantum mechanics is the continuous spontaneous localization (CSL) model76,77. It augments the Schrödinger equation for elementary particles with a Gaussian noise term that gives rise to a continuous stochastic collapse of wavefunctions delocalized beyond about 100 nm. The origin of the stochastic process remains unspecified; one may view it either as a fundamental trait of nature, or as the repercussion of an inaccessible underlying dynamics 78. The CSL effect would be very weak and practically unobservable on the atomic level, but it would get strongly amplified for bound atoms forming a solid, such as the pointer of a measurement device. Any superposition of macroscopically distinct positions would rapidly collapse, in agreement with Born’s rule, to a ‘classical’ state characterized by a localized, objective wavefunction. This way the model serves its purpose of restoring objective classical reality on the scale of everyday objects, allowing one to dispense with the measurement postulate.
It is a contentious issue whether such macrorealism79 is required in a plausible description of physical reality. Independent of that, the CSL model serves as a cautionary tale. It proves that there are competing descriptions of nature, which predict strongly different effects at macroscopic scales, even though they are compatible with all experiments and cosmological observations carried out so far71,80. One may invoke metaphysical arguments in favour of one or another theory, but empirically their status is equal, and only future experiments will be able to tell them apart.
Venturing towards macroscopic quantum superpositions
Various different systems have been suggested for probing the quantum superposition principle at mesoscopic or even macroscopic scales. This raises the question how to objectively assess the degree of macroscopicity reached in different experiments40 (Box 1).
The gravitational collapse hypothesis81 inspired a proposal to create a quantum superposition in the centre-of-mass motion of a micromirror82 (Fig. 3a). A lightweight (picogram) mirror suspended from a cantilever can close a cavity acting as one arm of a Michelson interferometer. A single photon entering the interferometer excites a superposition of the two cavity modes. The radiation pressure of the single photon induces a deflective oscillation of the small mirror by approximately the width of the zero-point motion. Which-path information is thus left behind once the photon escapes from the cavities, unless this occurs at a multiple of the cantilever oscillation period, when the original state of the mirror reappears. Observing the recurrence of optical interference after one such oscillation period would therefore prove that the mirror was in a superposition state82,83.
This is a difficult experiment because a relatively massive oscillator with an eigenfrequency in the low kilohertz regime is required for probing gravitational collapse. This implies that the oscillator ground state is reached only at microkelvin temperatures. Ground-state cooling is easier with lighter and more rigid megahertz or gigahertz oscillators, and by addressing normal modes with stronger opto-mechanical coupling. This feat has been achieved recently with the flexural mode of a circular aluminium micro-membrane using optical side-band cooling84,85. Many groups worldwide have embarked on studying such nanomechanical oscillators86, which can serve as an interface between quantum systems. However, it has been difficult to observe genuine quantum effects in optomechanical systems because they still lack the strong nonlinear coupling required to generate quantum states of motion that differ qualitatively from classical ones. As a first step in this direction a piezoelectric resonator was coupled coherently to a superconducting loop87.
The distinctive feature of micromechanical devices compared with other quantum systems is their very high mass. However, the quantum delocalization of the oscillatory ground state, which is a collective degree of freedom involving all the atoms, will reach at most about one picometre in conceivable set-ups—a tiny fraction of the size of an atom. This indicates why some matter-wave experiments will reach beyond the macroscopicity of a possible superposition of the micro-membrane (Box 1).
As any clamped nanostructure will be prone to damping, recent proposals88,89,90 consider levitating dielectric nanoparticles in the focus of an intense laser beam. Cooling the centre-of-mass motion to the ground state should be feasible, owing to their lower mass and the high trap frequencies. Moreover, the nanosphere position can be coupled nonlinearly to a resonator light field by placing the optical trap at the node of a Fabry–Pérot cavity. This opens the possibility to create distinctively non-classical states, and to probe the wave nature of the nano-spheres, for example, by implementing an effective double-slit91. In this scheme one would drop the nanosphere once it has been cooled to the ground state of a dipole trap. After the wave packet is sufficiently dispersed, a laser pulse passing through a Fabry–Pérot cavity reveals the square of the position by a homodyne measurement of the cavity light field. One thus learns the distance of the sphere from the cavity centre, but not whether it is on the left or right, thus effectively projecting its wavefunction to a spatial superposition state. An interference pattern should then be observable after a further free evolution of the sphere, and after many repetitions, if one correlates the detected positions with the results of the homodyne measurements (Fig. 3b). The nanosphere position would be delocalized by approximately the diameter of the sphere, which should be sufficiently large to test the effects of the CSL collapse model.
A straightforward strategy for probing the wave nature of nanometre-sized objects is to push established matter-wave interference schemes to the limits of large masses. The OTIMA interferometer (Fig. 3c) should allow us to probe the quantum nature of 105amu particles if the source ejects them with a velocity of about 10 m s−1 (ref. 53). Objects with a diameter up to 10 nm would get delocalized over 80 nm. In the future, even nanoparticles in the mass range of 108amu might be diffracted with an OTIMA scheme, for example gold clusters with a diameter of 22 nm. Successful interference at these masses would falsify all current CSL predictions52. However, it would require us to counteract the gravitational acceleration, by noise-free levitation techniques or by going to a microgravity environment, to allow the wavefunction to expand over a coherence time of many seconds. Moreover, environmental decoherence would need to be suppressed by setting the ambient pressure to below 10−11 mbar and by cooling the apparatus to cryogenic temperatures92; (Fig. 2). The biggest challenge, both for OTIMA interferometry and the realization of a projective double slit, is the preparation of size-selected neutral particles in ultra-high vacuum at low internal and motional temperatures. Some promising first steps have been achieved by recent demonstrations of optical feedback cooling93,94 and cavity cooling46,47.
Will the quantum superposition principle stand the test of time? We have emphasized that this question is neither crazy nor heretical. Objective modifications of quantum mechanics can be set up that agree with all observations and experiments so far, while describing a tangible breakdown of quantum theory at the macroscale. Whether quantum mechanics is universally valid is thus not an issue of conviction or metaphysical reasoning, but an empirical question, to be answered only by future experiments.
A great variety of quantum systems may be used to demonstrate mechanical superposition states, whose mass, geometric size and delocalization scales may vary by orders of magnitude. Any such quantum test, if carried out successfully, will rule out a generic class of objective modifications of quantum mechanics. Using the scope of this falsified class as a yardstick, it is remarkable that totally different experimental approaches lead to comparable degrees of macroscopicity This suggests that there is no single golden strategy to be pursued, and much will depend on experimental advances and ideas. It is thus a long and exciting journey into the realm of large quantum superpositions, and one worth taking.
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We thank S. Nimmrichter for helpful discussions, and we acknowledge support by the European Commission within NANOQUESTFIT (No. 304886). M.A. is supported by the Austrian FWF (Wittgenstein Z149-N16) and by the ERC (AdvG 320694 Probiotiqus), K.H. by the DFG (HO 2318/4-1 and SFB/TR12). We thank the WE Heraeus Foundation for supporting the physics school ‘Exploring the Limits of the Quantum Superposition Principle’.
The authors declare no competing financial interests.
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Arndt, M., Hornberger, K. Testing the limits of quantum mechanical superpositions. Nature Phys 10, 271–277 (2014). https://doi.org/10.1038/nphys2863
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